Abstract
Magnetic field dipolarizations are often observed in the magnetotail during substornis. These generally include three temporal scales: (1) actual dipolarization when the normal magnetic field changes during several minutes from minimum to maximum level;(2) sharp B-z bursts (pulses) interpreted as the passage of multiple dipolarization fronts with characteristic time scales < 1 min, and (3) bursts of electric and magnetic fluctuations with frequencies up to electron gyrofrequency occurring at the smallest tune scales (<= 1 s). We present a numerical model where the contributions of the above processes (1)-(3) in particle acceleration are analyzed. It is shown that these processes have a resonant character at different temporal scales. While O+ ions are more likely accelerated due to the mechanism (1), H+ ions (and to some extent electrons) are effectively accelerated due to the second mechanism. High-frequency electric and magnetic fluctuations accompanying magnetic dipolarization as in (3) are also found to efficiently accelerate electrons.
Dokumententyp: | Zeitschriftenartikel |
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Fakultät: | Geowissenschaften > Department für Geo- und Umweltwissenschaften |
Themengebiete: | 500 Naturwissenschaften und Mathematik > 550 Geowissenschaften, Geologie |
URN: | urn:nbn:de:bvb:19-epub-67868-6 |
ISSN: | 1593-5213 |
Sprache: | Englisch |
Dokumenten ID: | 67868 |
Datum der Veröffentlichung auf Open Access LMU: | 19. Jul. 2019, 12:23 |
Letzte Änderungen: | 04. Nov. 2020, 13:50 |